Orion ASTROVIEW 9862 User Manual
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What to Expect
So what will you see with your telescope? You should be able 
to see bands on Jupiter, the rings of Saturn, craters on the 
moon, the waxing and waning of Venus, and possibly hun-
dreds of deep sky objects. Do not expect to see as much color 
as you in NASA photos, since those are taken with long-expo-
sure cameras and have “false color” added. Our eyes are not 
sensitive enough to see color in deep-sky objects except in a 
few of the brightest ones.
Remember that you are seeing these objects using your own 
telescope with your own eyes! The object you see in your 
eyepiece is in real-time, and not some conveniently provided 
image from an expensive space probe. Each session with 
your telescope will be a learning experience. Each time you 
work with your telescope it will get easier to use, and stellar 
objects will become easier to find. Take it from us, there is 
big difference between looking at a well-made full-color NASA 
image of a deep-sky object in a lit room during the daytime, 
and seeing that same object in your telescope at night. One 
can merely be a pretty image someone gave to you. The other 
is an experience you will never forget!
A. The Moon
With is rocky and cratered surface, the moon is one of the 
most interesting and easy subjects for your scope. The best 
time to view it is during its partial phases when shadows fall 
on the craters and canyon walls to give its features definition. 
While the full moon may look like a tempting target, it is actu-
ally the worst time for viewing! The light of a full moon is too 
bright and lacks any decent surface definition. 
Use an optional Moon filter to dim the Moon when it is very 
bright. It simply threads onto the bottom of the eyepiece (you 
must first remove the eyepiece from the focuser to attach the 
filter). You’ll find the Moon filter improves viewing comfort, and 
helps bring out the subtle features in the lunar surface.
B. The Planets
The planets don’t stay put like stars do, so you will have to 
refer to charts published monthly on our website, telescope.
com, or other astronomy references to locate them. Venus, 
Mars, Jupiter, and Saturn are the brightest objects in the sky 
after the Sun and the Moon. All four of these planets are not 
normally visible in the sky at one time, but chances are one or 
two of them will be. Other planets will also be visible at times, 
but will appear star-like when viewed through your telescope.
JUPITER The largest planet, Jupiter, is a great subject to 
observe. You can see the disk of the giant planet and watch 
the ever-changing positions of its four largest moons, Io, 
Callisto, Europa, and Ganymede. If atmospheric conditions 
are good, you may be able to resolve thin cloud bands on the 
planet’s disk.
SATURN The ringed planet is a breathtaking sight when it is 
well positioned. The tilt angle of the rings varies over a period 
of many years; sometimes they are seen edge-on, while at 
other times they are broadside and look like giant “ears” on 
each side of Saturn’s disk. A steady atmosphere (good see-
ing) is necessary for a good view. You may see a tiny, bright 
“star” close by; that’s Saturn’s brightest moon, Titan.
VENUS At its brightest, Venus is the most luminous object in 
the sky, excluding the Sun and the Moon. It is so bright that 
sometimes it is visible to the naked eye during full daylight! 
Ironically, Venus appears as a thin crescent, not a full disk, 
when at its peak brightness. Because it is so close to the Sun, 
it never wanders too far from the morning or evening horizon. 
No surface markings can be seen on Venus, which is always 
shrouded in dense clouds.
MARS If atmospheric conditions are good, you may be able 
to see some subtle surface detail on the Red Planet, possibly 
even the polar ice cap. Mars makes a close approach to Earth 
every two years; during those approaches its disk is larger 
and thus more favorable for viewing.
C. The Sun
You can change your nighttime scope into a daytime Sun view-
er by installing an optional full-aperture solar-filter over the 
front opening of the AstroView 100 EQ. The primary attraction 
is sunspots, which change in shape, appearance, and location 
daily. Sunspots are directly related to magnetic activity in the 
sun and follow an 11 year cycle. Many observers like to make 
drawings of sunspots to monitor how the sun is changing from 
day to day.
Important Note: Do not look at the Sun with any optical 
instrument without a professionally made solar filter, or 
permanent eye damage could result. Also remember to 
cover or remove the finder scope before attempting to 
view the sun. 
D. Stars
Stars will appear like twinkling points of light in the telescope. 
Even the largest telescopes cannot magnify stars to appear 
as anything more than points of light! You can, however, enjoy 
the different colors of the stars and locate many pretty double 
and multiple stars. The famous “Double-Double” in the con-
stellation Lyra and the gorgeous two-color double star Albireo 
in Cygnus are favorites. Defocusing the image of a star slightly 
can help bring out its color.
E. Deep-Sky Objects
Under dark skies, you can observe a number of brighter deep-
sky objects with your AstroView 100 EQ, including gaseous 
nebulas, open and globular star clusters, and the brighter gal-
axies. Most deep-sky objects are very faint, so it is important 
that you find an observing site well away from light pollution. 
Take plenty of time to let your eyes adjust to the darkness. 
As you become more experienced and your observing skills 
improve, you will be able to coax out more and more intricate 
details. 
Finding Deep‑sky objects: starhopping
Starhopping, as it is called by astronomers, is perhaps the sim-
plest way to hunt down objects to view in the night sky. It entails 
first pointing the telescope at a star close to the object you wish to 
observe, and then progressing to other stars closer and closer to 
the object until it is in the field of view of the eyepiece. It is a very 
intuitive technique that has been employed for hundreds of years 
by professional and amateur astronomers alike. Keep in mind, 
